Results 41 to 50 of about 2,514,674 (303)

3D Solar Irradiance Model for Non-Uniform Shading Environments Using Shading (Aperture) Matrix Enhanced by Local Coordinate System

Energies, 2023
Building-integrated photovoltaics (BIPVs) and vehicle-integrated photovoltaics (VIPVs) receive solar irradiance through non-uniform shading objects. Standard scalar calculations cannot accurately determine the solar irradiance of BIPV and VIPV systems ...
Kenji Araki, Yasuyuki Ota, Akira Nagaoka, Kensuke Nishioka   +3 more
doaj   +1 more source

A multi-objective optimization model for the coordinated operation of hydropower and renewable energy

Frontiers in Energy Research, 2023
The rapid growth of wind and solar energy sources in recent years has brought challenges to power systems. One challenge is surging wind and solar electric generation, understanding how to consume such generation is important.
Benxi Liu, Zihan Peng, Shengli Liao, Tengyuan Liu, Jia Lu   +4 more
doaj   +1 more source

Seismology of the Standard Solar Model: Tests of Diffusion and the OPAL and MHD Equations of State [PDF]

, 1996
D. B. Guenther, Y.-C. Kim, P. Demarque
openalex   +2 more sources

The Neutrino Flux from an Updated Standard Solar Model [PDF]

Monthly Notices of the Royal Astronomical Society, 1975
A. Bolton
openalex   +3 more sources

Are Standard Solar Models Reliable? [PDF]

Physical Review Letters, 1997
4 pages, latex file. Revised numbers for Table 1.
Sarbani Basu, John N. Bahcall, Marc H. Pinsonneault, Jørgen Christensen-Dalsgaard   +3 more
openaire   +3 more sources

Solar response in tropical stratospheric ozone: a 3-D chemical transport model study using ERA reanalyses [PDF]

Atmospheric Chemistry and Physics, 2011
We have used an off-line 3-D chemical transport model (CTM) to investigate the 11-yr solar cycle response in tropical stratospheric ozone. The model is forced with European Centre for Medium-Range Weather Forecasts (ECMWF) (re)analysis (ERA-40 ...
S. Dhomse, M. P. Chipperfield, W. Feng, J. D. Haigh   +3 more
doaj   +1 more source

Using the standard solar model to constrain solar composition and nuclear reaction S factors [PDF]

, 2012
A. M. S. is partially supported by the European Union International Reintegration No. PIRG-GA-2009-247732, the MICINN Grant No. AYA2011-24704, by the ESF EUROCORES Program EuroGENESIS (MICINN Grant No.
A. Serenelli, C. Peña-Garay, W. Haxton
semanticscholar   +1 more source

Standard Solar Neutrinos [PDF]

Astrophys.J. 468 (1996) 933-946, 1996
An improved standard solar model has been used to calculate the fluxes of standard solar neutrinos. It includes premain sequence evolution, element diffusion, partial ionization effects, and all the possible nuclear reactions between the main elements. It uses updated values for the initial solar element abundances, the solar age, the solar luminosity,
arxiv   +2 more sources

Constraints on flavor-diagonal non-standard neutrino interactions from Borexino Phase-II

Journal of High Energy Physics, 2020
The Borexino detector measures solar neutrino fluxes via neutrino-electron elastic scattering. Observed spectra are determined by the solar-ν e survival probability P ee (E), and the chiral couplings of the neutrino and electron. Some theories of physics
The Borexino collaboration, S. K. Agarwalla, M. Agostini, K. Altenmüller, S. Appel, V. Atroshchenko, Z. Bagdasarian, D. Basilico, G. Bellini, J. Benziger, D. Bick, G. Bonfini, D. Bravo, B. Caccianiga, F. Calaprice, A. Caminata, L. Cappelli, P. Cavalcante, F. Cavanna, A. Chepurnov, K. Choi, D. D’Angelo, S. Davini, A. Derbin, A. Di Giacinto, V. Di Marcello, X. F. Ding, A. Di Ludovico, L. Di Noto, I. Drachnev, K. Fomenko, A. Formozov, D. Franco, F. Gabriele, C. Galbiati, M. Gschwender, C. Ghiano, M. Giammarchi, A. Goretti, M. Gromov, D. Guffanti, C. Hagner, E. Hungerford, Aldo Ianni, Andrea Ianni, A. Jany, D. Jeschke, S. Kumaran, V. Kobychev, G. Korga, T. Lachenmaier, M. Laubenstein, E. Litvinovich, P. Lombardi, L. Ludhova, G. Lukyanchenko, L. Lukyanchenko, I. Machulin, G. Manuzio, S. Marcocci, J. Maricic, J. Martyn, E. Meroni, M. Meyer, L. Miramonti, M. Misiaszek, V. Muratova, B. Neumair, M. Nieslony, L. Oberauer, V. Orekhov, F. Ortica, M. Pallavicini, L. Papp, Ö. Penek, L. Pietrofaccia, N. Pilipenko, A. Pocar, G. Raikov, G. Ranucci, A. Razeto, A. Re, M. Redchuk, A. Romani, N. Rossi, S. Rottenanger, S. Schönert, D. Semenov, M. Skorokhvatov, O. Smirnov, A. Sotnikov, C. Sun, Y. Suvorov, T. Takeuchi, R. Tartaglia, G. Testera, J. Thurn, E. Unzhakov, A. Vishneva, R. B. Vogelaar, F. von Feilitzsch, M. Wojcik, M. Wurm, O. Zaimidoroga, S. Zavatarelli, K. Zuber, G. Zuzel   +106 more
doaj   +1 more source

Higher metal abundances do not solve the solar problem [PDF]

A&A 669, L9 (2023), 2022
Context. The Sun acts as a cornerstone of stellar physics. Thanks to spectroscopic, helioseismic and neutrino flux observations, we can use the Sun as a laboratory of fundamental physics in extreme conditions. The conclusions we draw are then used to inform and calibrate evolutionary models of all other stars in the Universe.
arxiv   +1 more source